The Chemically Altered Basaltic Northern Plains of Mars: TES, OMEGA, and GRS Integrated Data Sets and Conclusions

Details The Chemically Altered Basaltic Northern Plains of Mars: TES, OMEGA, and GRS Integrated Data Sets and Conclusions The Chemically Altered Basaltic Northern Plains of Mars: TES, OMEGA, and GRS Integrated Data Sets and Conclusions

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3402w&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3402

Physics

Scientific paper

TES, OMEGA, and GRS data sets lead to the following conclusions: 1) the
northern plains are basaltic; 2) the basalt is chemically altered; and
3) the alteration likely resulted from surface interactions with
volatiles (snow) deposited during phases of high obliquity.

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